Result for 1005A381C3D27BBD35DC833A29577D341C46FA49

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.2.0/hawki_step_detect_obj.la
FileSize1033
MD5148D2ACB58C9E6784C29E61A3ACF761B
SHA-11005A381C3D27BBD35DC833A29577D341C46FA49
SHA-25610EBA5486A56A01D1127574C436FD7E657C4D66F511D26B081D3FA6719D5D0E4
SSDEEP24:PeSG1bWJU2icBxIY+Ahmfvi45vD2NGDe5/vp:lGVWJUzcBxIY1hmfKqLcvp
TLSHT19911AD3BD3DA613AAFD4194596CF313E4289847907312E5063C795DB224B81911A7E27
hashlookup:parent-total2
hashlookup:trust60

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Parents (Total: 2)

The searched file hash is included in 2 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize339148
MD5C58D5E032A626182ED9262A1DA69BDEA
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerUbuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1build1
SHA-1A3CF036AA00324958F4AD1F5F560ACB7C87F5FAE
SHA-25606CC17F274E65C368C62414C15C314154E9EE262D76EEC3AA890F81158595536
Key Value
FileSize412076
MD508B3CE36677FB07D89A49E60A807357C
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.2.0+dfsg-1+b1
SHA-1EDDFA8E4D2940474F63B25AC9BDAB2C9340BD1C7
SHA-256F5CDE157AB1385847031F916C70B8A0015D5F3794F32164E289FACCEFEA462DA